2013
DOI: 10.1103/physrevd.88.084043
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Matrix elements of Lorentzian Hamiltonian constraint in loop quantum gravity

Abstract: The Hamiltonian constraint is the key element of the canonical formulation of loop quantum gravity (LQG) coding its dynamics. In Ashtekar-Barbero variables it naturally splits into the so-called Euclidean and Lorentzian parts. However, due to the high complexity of this operator, only the matrix elements of the Euclidean part have been considered so far. Here we evaluate the action of the full constraint, including the Lorentzian part. The computation requires heavy use of SUð2Þ recoupling theory and several t… Show more

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Cited by 23 publications
(28 citation statements)
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“…Thanks to the calculation of the matrix elements of the volume operator in certain special case, some matrix elements of Thiemann's Hamiltonian constraint operator and its generalization were derived in [21,22]. Later on, the matrix elements was re-derived in [13], and then the formula in [13] was corrected by sign factors in [14,23] using graphical method. Matter coupling is also an important issue in LQG.…”
Section: Introductionmentioning
confidence: 99%
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“…Thanks to the calculation of the matrix elements of the volume operator in certain special case, some matrix elements of Thiemann's Hamiltonian constraint operator and its generalization were derived in [21,22]. Later on, the matrix elements was re-derived in [13], and then the formula in [13] was corrected by sign factors in [14,23] using graphical method. Matter coupling is also an important issue in LQG.…”
Section: Introductionmentioning
confidence: 99%
“…Brink's graphical method was only recalled in the appendix of [13]. Then Varshalovich's method was adopted in [14,23,28]. Brink's graphical method was also taken to study the propagator of spinfoam models in [29], in which the graphical method was only used to calculate the action of the right-invariant vector field (the "grasping operator") on the intertwiners but not the action of holonomy operator.…”
Section: Introductionmentioning
confidence: 99%
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“…It is defined employing a regularization procedure with specific rules that might be changed to bring it closer to the spinfoam formalism [17,18] (but till now spoiling the anomaly free property). However this operator is computationally extremely hard to implement [19], in particular its Lorentzian part which involves several commutators of the extrinsic curvature in order to express the Ricci scalar in terms of Holonomies and Fluxes. Few computations appeared so far [14,15] and few solutions have been found [16].…”
Section: Introductionmentioning
confidence: 99%